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Originally Posted by janoskiss
For best results the deconvolution algorithm should be told what the 'point spread function' of your instrument is. This can be deduced from aperture and central obstruction size: it is the Airy disk and diffraction rings you see when looking at stars at high powers.
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this bit steve, how do we tell the system the PSF. i know the aperture and central obstruction etc so what is the PSF for my scope?
work, whats work???